e-CALLISTO FITS Analyzer
Process and analyze e-CALLISTO dynamic spectra, isolate radio bursts, track their drift and estimate shock speeds and coronal magnetic fields.
Explore radio analysisFrom radio bursts to erupting coronal structures. Analyze e-CALLISTO spectra and solar images in one connected, open-source toolkit.

Start with a radio observation or an image sequence. Both tools come in the same free software package.
Process and analyze e-CALLISTO dynamic spectra, isolate radio bursts, track their drift and estimate shock speeds and coronal magnetic fields.
Explore radio analysisProcess and analyze solar imaging data from SDO, SOHO and STEREO through two complementary workspaces.
Process and analyze e-CALLISTO dynamic spectra, from the first FITS file to a publication-ready figure.
Subtract the background, tune display thresholds and clean radio-frequency interference from raw spectra.
Isolate features, extract intensity maxima and quantify drift, shock speed and Type II band splitting.
Bring GOES X-rays, CME catalogs, geomagnetic indices and solar imagery into the context of your observation.
Two connected workspaces bring solar images, measurements and three-dimensional CME fitting into your analysis. PFSS & GCS new in v3.1.0
Process and analyze SDO, SOHO and STEREO observations. Connect image sequences with CME measurements and magnetic-field context.

Fit a Graduated Cylindrical Shell to coronagraph images from multiple viewpoints. Evaluate CME geometry and propagation with a shared three-dimensional model.
Record fits, fit the shock separately, compare height–time evolution and export your fitting results.
Explore GCS fitting
Play examples exported from the Solar Image Analyzer and GCS tools.
Ridge tracking, five density models, multi-view GCS fitting, PFSS modelling and publication-style exports. Full release notes
The complete user guide covers every window, method and formula, from your first FITS file to three-dimensional CME reconstruction. Read it online or keep the PDF.
